October 31, 2014 Friday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) Informal Astro Talk Hendrik Eerten Max-Planck Institute Early time gamma-ray burst afterglows, thick shells and thin shells The afterglow signal following a gamma-ray burst often shows flat early time behavior in X-rays and optical that is distinct from the emission seen from 10^3 - 10^4 seconds onward, which more closely follows the expected decay for emission from a decelerating relativistic blast wave. In this talk I demonstrate how early time X- ray plateaus can be accounted for in thick shell' synchrotron models of prolonged energy injection, including the steep post-plateau decline in short bursts that is sometimes attributed to magnetar spindown. Studies of large samples of optical and X-ray afterglows also reveal a number of correlations between observables, most notably early period end times and optical / X-ray fluxes at that point. I show how these arise naturally from synchrotron emission in a thick shell model, but are hard to accommodate in a basic thin shell' model where the injected energy quickly ceases to leave an imprint on the blast wave structure and no relativistic reverse shock running through the ejecta develops. October 31, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee October 31, 2014 Friday 2:00 PM  + Meyer 5th Fl. CCPP Lounge Astrophysics and Relativity Seminars (astro) Alyson Brooks Rutgers University Re-Examining Astrophysical Constraints on the Dark Matter Model The cosmological model based on cold dark matter (CDM) and dark energy has been hugely successful in describing the observed evolution and large scale structure of our Universe. However, at small scales (in the smallest galaxies and at the centers of larger galaxies), a number of observations seem to conflict with the predictions CDM cosmology, leading to recent interest in Warm Dark Matter (WDM) and Self-Interacting Dark Matter (SIDM) models. These small scales, though, are also regions dominated by the influence of baryons. I will present results from high resolution cosmological galaxy simulations that include both baryons and dark matter to show that baryonic physics can significantly alter the dark matter structure and substructure of galaxies, revolutionizing our expectations for galaxy structure and influencing our interpretation of the Dark Matter model. November 3, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag November 4, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 5, 2014 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Jay Wacker Quora/Stanford University From Squarks to Startups, From Quarks to Quora November 5, 2014 Wednesday 2:00 PM  + Meyer 6th Floor Conference Room Soft Condensed Matter Seminars (csmr) Alex Mogilner Courant, New York University Motility initiation, turning and direction sensing in cells Animal cells crawl on flat surfaces using lamellipodium – dynamic network of actin polymers and myosin motors enveloped by the cell membrane. From the physical point of view, this network is an active contractile gel. Experimental analysis of the lamellipodial geometry, cell speed and actin dynamics in fish keratocyte cells combined with computational modeling suggested that steady crawling of the motile cells is based on two mechanisms: “actin treadmill inside unstretchable membrane bag” and “graded actomyosin contraction”. However, explanation of unsteady movements, especially of motility initiation and turning, remains elusive. I will present simulations of a 2D model of viscous contractile actin-myosin network with free boundary that, coupled with experimental data, suggests that stick-slip nonlinear adhesion is the key to understanding polarization and turning of the motile cells. Furthermore, we found that cells polarize very fast in electric field. Cytoplasmic fragments of fish keratocytes move to anode in electric field, while whole cells migrate to cathode. I will discuss implications of these finding for direction sensing mechanisms. November 6, 2014 Thursday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Mikhail Shifman University of Minnesota New exact results in supersymmetric theories at strong coupling November 6, 2014 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Zvonimir Dogic Brandeis University Autonomous Motility in Soft Active Matter The laws of equilibrium statistical mechanics impose severe constraints on the properties of conventional materials assembled from inanimate building blocks. Consequently, such materials cannot exhibit spontaneous motion or perform macroscopic work; i.e., a fluid in a beaker remains quiescent unless driven by external forces. Inspired by biological phenomena such Drosophila cytoplasmic streaming, our goal is to develop soft active materials assembled from animate, energy-consuming building blocks. Released from the constraints of the equilibrium, such internally driven materials are able to change-shape, oscillate, crawl, flow, swim, and exert forces on their boundaries to produce macroscopic work. They can serve as a platform for developing novel material applications, testing fundamental theoretical models of far-from-equilibrium active matter and potentially even shedding light on self-organization processes that take place in living cells. November 7, 2014 Friday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) Informal Astro Talk Tsvi Piran Hebrew University Gamma Ray Bursts and Life As a copious source of gamma-rays, a nearby Galactic Gamma-Ray Burst (GRB) can be a threat to life. Using recent determinations of the rate of GRBs, their luminosity function and properties of their host galaxies, we estimate the probability that a life-threatening (lethal) GRB would take place. Amongst the different kinds of GRBs, long ones are most dangerous. There is a very good chance (but no certainty) that at least one lethal GRB took place during the past 5 Gyr close enough to Earth as to significantly damage life. There is a 50% chance that such a lethal GRB took place during the last 500 Myr causing one of the major mass extinction events. Assuming that a similar level of radiation would be lethal to life on other exoplanets hosting life, we explore the potential effects of GRBs to life elsewhere in the Galaxy and the Universe. We find that the probability of a lethal GRB is much larger in the inner Milky Way (95% within a radius of 4 kpc from the galactic center), making it inhospitable to life. Only at the outskirts of the Milky Way, at more than 10 kpc from the galactic center, this probability drops below 50%. When considering the Universe as a whole, the safest environments for life (similar to the one on Earth) are the lowest density regions in the outskirts of large galaxies and life can exist in only ≈ 10% of galaxies. Remarkably, a cosmological constant is essential for such systems to exist. Furthermore, because of both the higher GRB rate and galaxies being smaller, life as it exists on Earth could not take place at z > 0.5. Early life forms must have been much more resilient to radiation. November 7, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 7, 2014 Friday 2:00 PM  + Meyer 5th Fl. CCPP Lounge Astrophysics and Relativity Seminars (astro) Esra Bulbul Harvard-Smithsonian Center for Astrophysics The curious case of the 3.57 keV Emission Line We recently detected an unidentified emission line at 3.57 keV in the Chandra observations of the Perseus cluster and the stacked XMM-Newton observations of 73 galaxy clusters. This line was detected at more than 3-sigma statistical significance in five independent samples of XMM-Newton. The lack of any atomic transitions at this energy in thermal plasma, hints that the line could be a signature of decaying sterile neutrinos. I will discuss the search for this line in the stacked observations of galaxy clusters and provide an update on active searches for this feature in other dark matter rich astrophysical systems. November 10, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag November 11, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 12, 2014 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) John Terning UC Davis TBA November 13, 2014 Thursday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) Informal Astro Talk Angela Burden Portsmouth Reconstruction of linear baryon acoustic oscillations TBA November 13, 2014 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Sharon Glotzer University of Michigan TBA November 14, 2014 Friday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) Informal Astro Talk Tsvi Piran Hebrew University To B or not to \vec{B} - the nature of GRBs and AGNS jets Will report studies of the propagation of magnetic (B with an arrow) or baryonic (B) jets in a dense medium and the implications for GRB and AGN jets. November 14, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 14, 2014 Friday 2:00 PM  + Meyer 5th Fl. CCPP Lounge Astrophysics and Relativity Seminars (astro) James Guillochon Harvard-Smithsonian Center for Astrophysics A Dark Year for Tidal Disruption Events The disruption of a star by a supermassive black hole results in the initial production of an extended, extremely thin debris stream that winds repeatedly around the black hole, producing a three-dimensional figure of ellipses that share a common periapse distance. I will show that typical encounters generate streams that are so thin that even small relativistic precession corrections can induce deflections that prevent the streams from intersecting one another. Additionally, hydrodynamical simulations have demonstrated that energy is deposited very slowly via hydrodynamical processes alone, resulting in the liberation of very little gravitational binding energy in the absence of stream-stream collisions. This state persists until the streams are precessed into the spin plane of the black hole, which corresponds to dozens or even hundreds of orbits of the most bound material, meaning that there can be a "dark period" between the time of disruption and the transient that can last years. I'll show that because the streams dissipate little energy prior to circularizing, the luminosity of these flares (despite the delay) should still closely follow the original fallback rate. November 17, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag November 17, 2014 Monday 2:00 PM  + Meyer 6th Floor Conference Room Soft Condensed Matter Seminars (csmr) Kelly Aubertin CNRS and University Diderot, Paris Impact of a Mechanical or a Photochemical Stress on the Intracellular Trafficking The cell cytoplasm is crowded with membrane-delimited compartments, permanently exchanging with each other. Such exchange is permitted by active transport, also called intracellular trafficking, of vesicles along the cytoskeleton (actin filaments, microtubules), and mediated by molecular motors. In order to perturbate this intracellular trafficking, two different ways to apply controlled physical stresses have been performed. The first perturbation is a mechanical one: we used magnetic endosomes to apply a mechanical stress to the cell body and to probe the activity. To obtain them, we internalized magnetic nanoparticles into mesenchymal stem cells (MSC) through the natural endocytosis pathway. These endosomes align into chains in the presence of a magnetic field. The mechanical perturbation then consists in applying a rotational magnetic field on these chains. When comparing the activity before and after a shear stress, we observed a small decrease in the intracellular activity. The second perturbation has a photochemical origin, through the excitation of internalized photosensitizer molecules (m-THPC or TPCS2a) into prostatic cancer cells (PC3). By combining measurements of local cytoplasmic viscosity and intracellular activity, we found that the photo-activation induced only a slight increase in viscosity while a massive slowing down of trafficking was observed. These effects are correlated with the depolymerization of the microtubule network. The experiments demonstrate that these two photochemical agents have different intracellular impacts. Eventually, we studied a second effect of the photochemical perturbation which is the massive and rapid emission of extracellular vesicles directly after the treatment. November 18, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 19, 2014 Wednesday 2:00 PM  + Meyer 6th Floor Conference Room Soft Condensed Matter Seminars (csmr) Damon Clark TBA November 19, 2014 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Nemanja Kaloper November 20, 2014 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Richard Gaitskell Brown University TBA November 21, 2014 Friday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) Informal Astro Talk Yossi Shvartzvald Tel Aviv University Results from the OGLE-MOA-Wise Microlensing Survey The discovery of thousands of extrasolar planets ranks among the most exciting scientific developments of the past decade. Among the techniques currently used to discover extrasolar planets, microlensing has some unique capabilities. It is the most sensitive technique to detect planets beyond the "snowline", where gas and ice giants are likely to form. Starting April 2011, we have begun a "second generation" microlensing survey, combining OGLE, MOA, and the Wise observatory. I will present a preliminary statistical analysis for the first three seasons of the survey. Over 10% of the events that were observed by all three sites showed a deviation from a single-lens microlensing, and for almost 1/3 of those the anomaly might be explained by a planetary companion. By accounting for our detection efficiency, we find a ~20-25% planetary system abundance, which is in line with previous microlensing estimates. Moreover, our results suggests that massive planets around low-mass stars are common, which may be in conflict with planetary formation scenarios. The data also can set constraints on the multiplicity fraction and the binary mass ratio distribution. November 21, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 21, 2014 Friday 12:00 PM  + Other CCPP (ccpp) Big Apple Colloquium David Charbonneau Harvard-Smithsonian Center for Astrophysics November 24, 2014 Monday 11:00 AM  + Meyer 721 Hard Condensed Matter Seminars (hcmp) Chandra Varma University of California, Riverside Local Quantum-Criticality in the Dissipative XY-Model in 2D Quantum critical fluctuations in which the time-dependence is scale invariant but the spatial dependence is local stand in contrast to the paradigm of classical dynamical critical phenomena and its simple quantum generalization. There is experimental evidence for them near the quantum critical point both in cuprates and near the Anti-ferromagnetic critial point in Fe-based superconductors and in some heavy Fermions. The dissipative Quantum XY-Model, proposed initially to describe the superconductor to insulator transition in thin films, with an anisotropic generalization, describes both. I will summarize an analytical solution of the model which derives local quantum critical fluctuations for this model as due to the proliferation of a class of topological exciations and supplement it by Monte-Carlo calculations on the model. November 24, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag November 25, 2014 Tuesday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Astrophysics and Relativity Seminars (astro) Michael Kesden UT Dallas The gravitational-wave signatures of astrophysical binary black-hole formation Binary stars of sufficient mass can collapse into binary black holes at the end of their main-sequence evolution. These binary black holes emit gravitational waves that extract energy and angular momentum from their orbit, cauing the black holes to inspiral and eventually merge. Mass transfer and tidal alignment during the evolution of the black hole's stellar progenitors can induce an asymmetry in the misalignment of binary black-hole spins with the orbital angular momentum. If binaries preferentially form with the the spins of the more massive black hole more (less) aligned with the orbital angular momentum than that of the less massive black hole, the components of the spin in the orbital plane will preferentially align (anti-align) during the gravitational-wave induced inspiral. Once trapped in these spin-orbit resonances, the orbital angular momentum and both spins jointly precess in a common plane during the remainder of the inspiral. We examine the gravitational waves emitted by binary black holes in these resonant configurations, and find that binaries with aligned spin components in the orbital plane can be distinguished by the greater precession of the orbital plane. This precession leaves a distinctive signature in the gravitational waveform which can be identified by ground-based gravitational-wave detectors in sources with sufficient signal-to-noise ratios, allowing gravitational-wave observers to distinguish different scenarios for binary black-hole formation. November 25, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee November 28, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 1, 2014 Monday 11:00 AM  + Meyer 5th Fl. CCPP Lounge Experimental Particle Physics Seminars (hep-ex) Mark Cooke Lawrence Berkeley National Laboratory ... Naturalness and Searches for Vector-like Quarks with the ATLAS detector December 1, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag December 2, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 3, 2014 Wednesday 2:00 PM  + Meyer 6th Floor Conference Room Soft Condensed Matter Seminars (csmr) Maxime Clusel Stochastic Thermodynamics, From ħ=0 to ħ=1 Progress has been made during the last decades in the development of a statistical theory for classical out-of-equilibrium system. In addition to celebrated fluctuation theorems, stochastic thermodynamic now provides both a nice unifying theoretical framework and a useful way for studying these systems experimentally. It was for instance at the heart of the first experimental verification of Landauer principle. After reviewing the classical case, I will propose an attempt to construct a quantum stochastic thermodynamics based on a quantum trajectory description of driven open systems. This framework allows for definitions at the single trajectory level of basic thermodynamic quantities such as heat transfer, work and entropy in the quantum regime. It can then be used to obtained “central” fluctuation theorems, from which follow more"practical" fluctuation relations such as for instance Jarzynski and Crooks fluctuation theorems. I will discuss in particular similarities and differences between the ħ=0 and ħ=1 regimes. December 3, 2014 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Steen Hannestad Aarhus University December 4, 2014 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Paul Janmey University of Pennsylvania TBA December 5, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 5, 2014 Friday 2:00 PM  + Meyer 5th Fl. CCPP Lounge Astrophysics and Relativity Seminars (astro) Ori Fox Berkeley/NASA December 8, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag December 9, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 10, 2014 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Jared Kaplan Johns Hopkins University TBA December 11, 2014 Thursday 2:00 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) Other Physics Student Hour with Ali Yazdani December 11, 2014 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Ali Yazdani Princeton University TBA December 11, 2014 Thursday 5:30 PM  + Meyer 6th Floor CSMR Area Other Physics Department Events (other) Physics Department Holiday Party Light refreshments will be served. December 12, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 12, 2014 Friday 2:00 PM  + Meyer 5th Fl. CCPP Lounge Astrophysics and Relativity Seminars (astro) Christy Tremonti University of Wisconsin, Madison Constraining Galaxy Feeding and Feedback with MaNGA A central issue in galaxy evolution is understanding the "baryon cycle," namely how gas is accreted onto galaxies and expelled in galactic winds. Gas flows are difficult to measure directly, but disk galaxy nebular oxygen abundance measurements can provide powerful indirect constraints. I will present some early work form the SDSS-IV MaNGA survey which will obtain spatially resolved oxygen abundance measurements of around 5,000 disk galaxies. December 15, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag December 16, 2014 Tuesday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 17, 2014 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Christoph Uhlemann University of Washington TBA December 19, 2014 Friday 11:30 AM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) astro coffee December 22, 2014 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag Gia Dvali January 26, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag January 29, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Alessandra Lanzara UC Berkeley TBA February 2, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag February 4, 2015 Wednesday 2:00 PM  + Meyer 6th Floor Conference Room Soft Condensed Matter Seminars (csmr) Yitzhak Rabin Bar Ilan University TBD February 4, 2015 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Frederik Denef Columbia University TBA February 5, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) John Johnson TBA February 9, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag February 11, 2015 Wednesday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Albion Lawrence Brandeis TBA February 12, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Vincenzo Vitelli Leiden TBA February 16, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag February 23, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag February 26, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Vicky Kaspi McGill University TBA March 2, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag March 9, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag March 12, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Joe Lykken TBA March 16, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag March 23, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag March 26, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Jerome Bibette EPSCI TBA March 30, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag April 3, 2015 Friday 2:00 PM  + Meyer 5th Fl. CCPP Lounge High Energy Physics Seminars (hep) Adam Peterson University of Minnesota TBA April 6, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag April 9, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Mikhail Lukin Harvard University TBA April 13, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag April 16, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Gabriel Kotliar TBA April 20, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag April 27, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag April 30, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Marc Kamionkowksi TBA May 4, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag May 7, 2015 Thursday 4:00 PM  + Meyer 122 Physics Colloquia (colloquia) Steve Furlanetto TBA May 11, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag May 18, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag May 25, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag June 1, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag June 8, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag June 15, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag June 22, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag June 29, 2015 Monday 12:30 PM  + Meyer 5th Fl. CCPP Lounge Other CCPP (ccpp) CCPP Brown Bag